{ "id": "2002.11123", "version": "v1", "published": "2020-02-25T19:00:01.000Z", "updated": "2020-02-25T19:00:01.000Z", "title": "Diffusive shock acceleration in $N$ dimensions", "authors": [ "Assaf Lavi", "Ofir Arad", "Yotam Nagar", "Uri Keshet" ], "comment": "14 pages, 7 figures, comments welcome", "categories": [ "astro-ph.HE" ], "abstract": "Collisionless shocks are often studied in two spatial dimensions (2D), to gain insights into the 3D case. We analyze diffusive shock acceleration for an arbitrary number $N\\in\\mathbb{N}$ of dimensions. For a non-relativistic shock of compression ratio $\\mathcal{R}$, the spectral index of the accelerated particles is $s_E=1+N/(\\mathcal{R}-1)$; this curiously yields, for any $N$, the familiar $s_E=2$ (i.e., equal energy per logarithmic particle energy bin) for a strong shock in a mono-atomic gas. A precise relation between $s_E$ and the anisotropy along an arbitrary relativistic shock is derived, and is used to obtain an analytic expression for $s_E$ in the case of isotropic angular diffusion, affirming an analogous result in 3D. In particular, this approach yields $s_E = (1+\\sqrt{13})/2 \\simeq 2.30$ in the ultra-relativistic shock limit for $N=2$, and $s_E(N\\to\\infty)=2$ for any strong shock. The angular eigenfunctions of the isotropic-diffusion transport equation reduce in 2D to elliptic cosine functions, providing a rigorous solution to the problem; the first function upstream already yields a remarkably accurate approximation. We show how these and additional results can be used to promote the study of shocks in 3D.", "revisions": [ { "version": "v1", "updated": "2020-02-25T19:00:01.000Z" } ], "analyses": { "keywords": [ "dimensions", "isotropic-diffusion transport equation reduce", "logarithmic particle energy bin", "strong shock", "analyze diffusive shock acceleration" ], "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable" } } }